We have shown in our previous paper [1]} that the effects of EQG on the angular radius of the shadow of Sgr A* is less than 10 nanoarcseconds. Here we see that the same thing is also true for the angular positions of relativistic images. In this case the differential time delay between relativistic images could be used to test EQG, if (since they are highly demagnified) these images could ever be observed.
